Table D.1
Excerpt of the table summarising the properties of the K2 stars studied in this work.
| EPIC | G (mag) | GBP - GRP (mag) | MG (mag) | Prot (day) | Flag | Sph a (ppm) | log R′IRT | ρ̄ |
|---|---|---|---|---|---|---|---|---|
| 201094776 | 15.3 | 0.85 | 5.60 | 11.15 ± 3.00 | 1 | 1831 | – | –0.50 |
| 201097220 | 13.6 | 0.82 | 4.59 | 6.08 ± 1.05 | 0 | 4043 ± 85 | – | 0.25 |
| 201098208 | 14.8 | 1.29 | 6.59 | 13.04 ± 2.35 | 0 | 5827 | – | 0.20 |
| 201102172 | 16.2 | 2.43 | 10.05 | 3.45 ± –1.00 | 1 | 7464 ± 932 | – | 0.42 |
| 201103864 | 13.4 | 1.06 | 5.89 | 21.74 ± 4.99 | 1 | 4658 | – | 0.21 |
| 201114114 | 14.6 | 1.20 | 6.47 | 16.42 ± 4.29 | 0 | 1168 | – | 0.04 |
| 201116316 | 12.9 | 1.14 | 5.63 | 2.57 ± 0.45 | 1 | 15747 ± 7197 | – | 0.87 |
| 201121691 | 12.7 | 1.12 | 5.34 | 3.92 ±–1.00 | 1 | 8178 ± 2876 | – | 0.82 |
| 201123647 | 14.0 | 1.11 | 5.72 | 6.77 ± 1.10 | 0 | 15041 ± 2389 | – | 0.70 |
| 201131271 | 13.9 | 1.09 | – | 2.25 ± –1.00 | 1 | 7808 ± 1771 | – | 0.78 |
| 201132458 | 15.0 | 2.24 | – | 2.54 ± 0.38 | 1 | 14898 ± 1060 | – | 0.71 |
| 201134718 | 13.4 | 1.70 | 7.09 | 1.43 ± –1.00 | 1 | 8676 ± 1884 | – | 0.94 |
| 201140864 | 16.0 | 2.40 | 10.15 | 5.11 ± 0.82 | 1 | 19791 ± 927 | – | 0.33 |
| 201149128 | 15.9 | 2.40 | 10.04 | 2.02 ±–1.00 | 1 | 18889 ± 587 | – | 0.52 |
| 201154929 | 14.8 | 2.07 | 8.69 | 23.59 ± 4.98 | 1 | 4839 | – | 0.25 |
| 201166582 | 15.9 | 1.89 | 8.10 | 1.33 ± 0.21 | 1 | 2772 ± 928 | – | 0.30 |
| 201178569 | 15.8 | 2.42 | 9.57 | 2.70 ± 0.42 | 1 | 7211 ± 1013 | – | –0.10 |
| 201212507 | 14.6 | 1.58 | 7.58 | 11.33 ± 3.80 | 0 | 3994 | – | 0.21 |
| 201223827 | 15.8 | 1.16 | 6.60 | 1.86 ± –1.00 | 1 | 8634 ± 1354 | – | 0.18 |
| 201235266 | 12.5 | 1.22 | 6.44 | 23.20 ± 5.01 | 1 | 4031 | –5.4 | 0.50 |
| 201249315 | 14.9 | 1.13 | 6.17 | 2.70 ± 0.40 | 1 | 8163 ± 1781 | – | 0.82 |
| 201272989 | 14.3 | 1.58 | 7.48 | 16.16 ± –1.00 | 1 | 2293 ± 1264 | – | 0.24 |
| 201273096 | 14.9 | 1.33 | 6.45 | 14.95 ± 4.16 | 0 | 1724 | – | 0.24 |
| 201288384 | 10.8 | 1.78 | – | 5.30 ± 0.82 | 1 | 19583 ± 1776 | – | 0.80 |
| 201308300 | 11.8 | 0.75 | 4.46 | 4.48 ± 0.83 | 1 | 3121 ± 720 | –6.1 | 0.67 |
| 201346007 | 15.1 | 2.26 | 9.38 | 17.03 ± 3.27 | 0 | 8271 | – | 0.46 |
| 201366994 | 15.0 | 1.35 | 5.73 | 0.54 ± 0.08 | 1 | 11001 ± 1141 | – | 0.57 |
| 201377225 | 14.4 | 1.90 | 7.61 | 3.18 ± 0.47 | 1 | 16981 ± 2943 | – | 0.46 |
| 201378489 | 13.7 | 1.52 | 6.63 | 28.11 ± 12.10 | 0 | 2580 | – | –0.24 |
| 201383978 | 17.9 | 2.74 | – | 2.89 ± 1.13 | 1 | 2161 ± 625 | – | 0.01 |
Notes. The full version is available at the CDS. The Flag column indicates whether the stars belong to the K2-Gaia cross validate sample (1) or not (0). When possible, the Bp - Rp magnitudes are corrected with the Apsis dereddening coefficients. (a)The Sph activity index being computed on light curve segments of length min(tobs, 5 × Prot), with tobs the total observing time, we do not provide an uncertainty on Sph for targets for which the light curve is shorter than 5 × Prot. When possible, the Bp - Rp magnitudes are corrected with the Apsis dereddening coefficients.
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